Source: The Astrophysical Journal. Unidade: IAG
Subjects: PLANETAS, ABUNDÂNCIA ESTELAR, ESTRELAS
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ABNT
RAMÍREZ, I et al. Elemental abundance differences in the 16 Cygni binary system: a signature of gas giant planet formation?. The Astrophysical Journal, v. 740, p. 76/1-76/15, 2011Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/740/2/76. Acesso em: 13 set. 2024.APA
Ramírez, I., Meléndez Moreno, J. L., Cornejo, D., Roederer, I. U., & Fish, J. R. (2011). Elemental abundance differences in the 16 Cygni binary system: a signature of gas giant planet formation? The Astrophysical Journal, 740, 76/1-76/15. doi:10.1088/0004-637X/740/2/76NLM
Ramírez I, Meléndez Moreno JL, Cornejo D, Roederer IU, Fish JR. Elemental abundance differences in the 16 Cygni binary system: a signature of gas giant planet formation? [Internet]. The Astrophysical Journal. 2011 ; 740 76/1-76/15.[citado 2024 set. 13 ] Available from: https://doi.org/10.1088/0004-637X/740/2/76Vancouver
Ramírez I, Meléndez Moreno JL, Cornejo D, Roederer IU, Fish JR. Elemental abundance differences in the 16 Cygni binary system: a signature of gas giant planet formation? [Internet]. The Astrophysical Journal. 2011 ; 740 76/1-76/15.[citado 2024 set. 13 ] Available from: https://doi.org/10.1088/0004-637X/740/2/76
